Young stellar outflows near-IR imaging (Varricatt+ 2010)

Details Young stellar outflows near-IR imaging (Varricatt+ 2010) Young stellar outflows near-IR imaging (Varricatt+ 2010)

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..74040661v&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/404/661. Originally published in: 2010MNRAS.404..661V

Physics

Ysos, Infrared Sources

Scientific paper

These are images of Massive Young Stellar outflow candidates obtained using the United Kingdom Infrared Telescope (UKIRT) and UFTI (UKIRT Fast-Track Imager). The pixel scale is 0.091arcsec/pixel. Images obtained in broad band K (2.2um, MKO) filter and in narrow-band filters centered at the wavelengths of H2 (2.1218um) and BrGamma (2.166um) lines are given here. Sky conditions were either photometric or thin cirrus, as mentioned in the paper. The mosaics presented here are ~2.2x2.2arcmin2^ across. The images are not flux calibrated. The images in the three filters, with names ending with "_K.fit", "H2.fit" or "BrG.fit" have the exposure time defined in the fits keyword "EXPTIME". For H2_ and BrGamma, images after normalization (to 1sec exposure time) and continuum-subtraction (with scaled K-band images) are also presented. The names of these images end in "norcs.fit".
(3 data files).

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